DESI installation: preparations and progress (Conference Presentation)
DESI installation: preparations and progress (Conference Presentation)
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DESI安装：准备和进展（会议演示）
DOI：
10.1117/12.2312159
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发表时间：
2018
期刊：
影响因子：
--
通讯作者：
T. O'Brien
中科院分区：
文献类型：
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作者：
L. Allen;D. Sprayberry;M. Evatt;R. Marshall;B. Abareshi;T. Lavoie;R. R. Joyce;R. Probst;A. Dey;R. Blum;R. Besuner;P. Jelinsky;J. Silber;T. Claybaugh;C. Poppett;P. Doel;D. Brooks;G. Gutiérrez;B. Flaugher;G. Gallo;D. Friend;R. Sharples;D. Bramall;K. Honscheid;P. Martini;M. Derwent;T. O'Brien
暗能量光谱仪(DESI)正在建造中，以使用重子声振荡技术测量宇宙的膨胀历史。在实验期间，将测量超过14000平方度的3,500万个星系和类星体的光谱。*KPNO Mayall望远镜的新主焦校正器将向5000个光纤定位器提供光。这些纤维依次供给十台宽带光谱仪。我们将介绍马亚尔望远镜及其周围环境为联合国可持续发展教育十年所做的大量准备工作，并将报告安装可持续发展教育十年本身的最新进展情况。
The Dark Energy Spectroscopic Instrument (DESI) is under construction to measure the expansion history of the Universe using the Baryon Acoustic Oscillation technique. The spectra of 35 million galaxies and quasars over 14000 sq deg will be measured during the life of the experiment. A new prime focus corrector for the KPNO Mayall telescope will deliver light to 5000 fiber optic positioners. The fibers in turn feed ten broad-band spectrographs. We will describe the extensive preparations of the Mayall telescope and its environs for DESI, and will report on progress-to-date of the installation of DESI itself.